antiquated
发表于 2025-3-26 23:48:32
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maroon
发表于 2025-3-27 03:24:21
Observations of Coronal Mass Ejections with the Coronal Multichannel Polarimeter,, CoMP observations provide high-cadence image sequences of the coronal line intensity, Doppler shift, and line width simultaneously over a large field of view. By studying the Doppler shift and line width we may explore more of the physical processes of the initiation and propagation of coronal mas
偶然
发表于 2025-3-27 07:56:00
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jet-lag
发表于 2025-3-27 13:24:12
3D Coronal Density Reconstruction and Retrieving the Magnetic Field Structure during Solar Minimum,EREO/COR1 data obtained during a deep minimum of solar activity in February 2008 (Carrington Rotation CR 2066) to retrieve and analyze the three-dimensional (3D) coronal electron density in the range of heights from 1.5 to 4 R. using a tomography method. With this, we qualitatively deduced structure
tenosynovitis
发表于 2025-3-27 17:28:05
,Photospheric Magnetic Field: Relationship Between North–South Asymmetry and Flux Imbalance,egion were taken into account. The north–south asymmetry of the magnetic fluxes was considered as well as the imbalance between positive and negative fluxes. The north–south asymmetry displays a regular alternation of the dominant hemisphere during the solar cycle: the northern hemisphere dominated
Surgeon
发表于 2025-3-27 21:44:52
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职业
发表于 2025-3-28 00:57:41
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无脊椎
发表于 2025-3-28 02:26:15
A Reconstruction of Ultraviolet Spectral Irradiance During the Maunder Minimum,ressed magnetic activity spanning the second half of the 17th century. This spectral reconstruction is based on an extension of the Monte Carlo Solar Spectral Irradiance Model (MOCASSIM). The new version of the model, documented in this paper, extends its spectral range down to 150 nm, its temporal
新娘
发表于 2025-3-28 09:20:01
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得罪
发表于 2025-3-28 12:10:43
3D Coronal Density Reconstruction and Retrieving the Magnetic Field Structure during Solar Minimum,EREO/COR1 data obtained during a deep minimum of solar activity in February 2008 (Carrington Rotation CR 2066) to retrieve and analyze the three-dimensional (3D) coronal electron density in the range of heights from 1.5 to 4 R. using a tomography method. With this, we qualitatively deduced structure